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Hossein Azizi

Hossein Azizi

Academic rank: Professor
ORCID:
Education: PhD.
ScopusId: 56186773800
Faculty: Faculty of Engineering
Address:
Phone: 0871-6660073

Research

Title
Geochronological and geochemical constraints on the petrogenesis of high-K granite from the Suffi abad area, Sanandaj-Sirjan Zone, NW Iran
Type
JournalPaper
Keywords
Sanadaj-Sirjan Zone High-K granite I-type granite Sr–Nd isotopes U–Pb zircon age
Year
2011
Journal Chemie der Erde-Geochemistry
DOI
Researchers Hossein Azizi ، YoshiHero Asaha ، behzad Mehrabi ، Soon Linchang

Abstract

The Sanandaj-Sirjan Zone (SSZ) trends northwestward in western Iran on the Precambrian to Paleozoic basement and exposes abundant I-type granitoids and calc-alkaline volcanic rocks that were most active during the Late Jurassic to Upper Cretaceous. The petrogenesis of the granitoids and associated volcanic rocks has been widely related to Neotethyan subduction beneath the Iranian plate. We report a geochronological and geochemical study of the Suffi abad granite (SLG) body that crops outs southeast of Sanandaj within the SSZ and is mainly composed of K-feldspar + quartz + plagioclase±hornblende. The SLG, which shows a high-K calc-alkaline affinity, has LA-ICPMS zircon U–Pb ages ranging between 149±2 and 144±3Ma and initial 87Sr/86Sr of∼0.7024–0.7069 and 143Nd/144Ndof∼0.5125–0.5127. These value correspond to an εNd (145 Ma) of +1.5 and +4.9, suggesting that the SLG originated from the juvenile crust or depleted mantle with a young TDM (650–900 Ma) over the subduction zone beneath the SSZ. Zircon saturation temperatures suggest that crystallization of the zircons, or emplacement of the host magmas, occurred at 560–750 ◦C, consistent with an intergrowth texture of K-feldspar and quartz that implies crystallization around the K-feldspar-quartz eutectic at lower temperatures. Overall, geochemical data suggest that crystallization of the hornblende and plagioclase played a role in magma differentiation. These data allow us to conclude that the high-K SLG did not originate directly from the juvenile mantle source as do most I-type, calc-alkaline granitoids, but more likely was produced from the partial melting of pre-existing I-type granitoids in the upper continental crust under low pressure conditions.